Design of Equilateral Array Polygonal Gravitational-Wave Observatory Formation near Lagrange Point <i>L</i><sub>1</sub>—Equilateral Triangle and Equilateral Tetrahedral Configurations

Design of Equilateral Array Polygonal Gravitational-Wave Observatory Formation near Lagrange Point <i>L</i><sub>1</sub>—Equilateral Triangle and Equilateral Tetrahedral Configurations

To observe lower-frequency gravitational waves (GWs), it is effective to utilize a large spacecraft formation baseline, spanning hundreds of thousands to millions of kilometers. To overcome the limitations of a gravitational-wave observatory (GWO) on specific orbits, a scientific observation mode an...

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Bibliographic Details
Main Authors: Zhengxu Pan, Mai Bando, Zhanxia Zhu, Shinji Hokamoto
Format: Article
Language:English
Published: MDPI AG 2024-12-01
Series:Aerospace
Subjects:
two observation modes
equilateral triangle array formation
equilateral tetrahedral array formation
gravitational-wave observatory
output regulation theory
Online Access:https://www.mdpi.com/2226-4310/11/12/1048
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